Tipo de publicación: Con árbitro

  • Publicación
    The PAU Survey and Euclid: Improving broadband photometric redshifts with multi-task learning
    Current and future imaging surveys require photometric redshifts (photo-zs) to be estimated for millions of galaxies. Improving the photo-z quality is a major...
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    The PAU survey: classifying low-z SEDs using Machine Learning clustering
    We present an application of unsupervised Machine Learning clustering to the PAU survey of galaxy spectral energy distribution (SED) within the COSMOS field...
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    The PAU Survey: Galaxy stellar population properties estimates with narrowband data
    A newfound interest has been seen in narrowband galaxy surveys as a promising method for achieving the necessary accuracy on the photometric redshift estimate...
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    The PAU survey: photometric redshift estimation in deep wide fields
    We present photometric redshifts (photo-z) for the deep wide fields of the Physics of the Accelerating Universe Survey (PAUS), covering an area of $\sim$50 deg...
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    The PDS 110 observing campaign - photometric and spectroscopic observations reveal eclipses are aperiodic
    PDS 110 is a young disc-hosting star in the Orion OB1A association. Two dimming events of similar depth and duration were seen in 2008 (WASP) and 2011 (KELT)...
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    The peculiar Balmer line profiles of OQ 208
    Spectrophotometric observations of OQ 208 over the time period between March 1985 and February 1991 are presented. It is found that the H-beta flux varies...
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    The peculiar chemical abundance of the transitional millisecond pulsar PSR J1023+0038 - Li enhancement
    Using high-resolution optical spectroscopy we determine the chemical abundance of the secondary star in the binary millisecond pulsar PSR J1023+0038. We measure...
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    The peculiar nature of BD + 24 deg 676
    The H-alpha emission star BD + 24 deg 676, formerly classified as a T Tauri star and more recently as a Herbig Ae star, has been observed at moderately high...
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    The Peculiar Optical Spectrum of 4C+22.25: Imprint of a Massive Black Hole Binary?
    We report the discovery of peculiar features in the optical spectrum of 4C+22.25, a flat spectrum radio quasar at z = 0.4183 observed in the Sloan Digital Sky...